2016MNRAS.458.1660L

Query : 2016MNRAS.458.1660L

2016MNRAS.458.1660L - Mon. Not. R. Astron. Soc., 458, 1660-1670 (2016/May-2)

Observationally constraining gravitational wave emission from short gamma-ray burst remnants.

LASKY P.D. and GLAMPEDAKIS K.

Abstract (from CDS):

Observations of short gamma-ray bursts indicate ongoing energy injection following the prompt emission, with the most likely candidate being the birth of a rapidly rotating, highly magnetized neutron star. We utilize X-ray observations of the burst remnant to constrain properties of the nascent neutron star, including its magnetic field-induced ellipticity and the saturation amplitude of various oscillation modes. Moreover, we derive strict upper limits on the gravitational wave emission from these objects by looking only at the X-ray light curve, showing the burst remnants are unlikely to be detected in the near future using ground-based gravitational wave interferometers, such as Advanced LIGO.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): gravitational waves - gamma-ray burst: general - stars: neutron

CDS comments: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 Fermi bn080905499 G 19 10 42.0450 -18 52 54.510           ~ 200 0
2 GRB 051221 G 21 54 48.626 +16 53 27.16 19.49         ~ 377 0
3 GRB 061201 gB 22 08 32.060 -74 34 47.90           ~ 205 0

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